[vsnet-outburst 9184] V601 Sco outburst? ID?

[Taichi Kato]

   According to ASAS-3 data, V601 Sco (UG:) relatively regularly
brightens to V ~13.3 (period about 40 d).  Is this true V601 Sco
or contamination of a nearby star?

   It is reported bright now.  Confirmation of the brightened object
might be helpful in resolving the identity.

  YYYYMMDD(UT)   mag  observer
  20080702.1150 <14.50V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20080702.1596 <14.50V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20080704.1403 <14.50V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20080704.1667 <14.50V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20080706.1680 13.607V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20080708.1003 13.494V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20080708.1115 13.421V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20080710.1415 13.167V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))
  20080710.1513 13.515V  (ASAS (Pojmanski, G. 2002, Acta Astron. 52,397))